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space-iconSpace and Physics
clock-iconPUBLISHEDSeptember 16, 2016

Some Martian Lakes Formed Much Later Than We Expected

Dr. Alfredo Carpineti headshot

Dr. Alfredo Carpineti

Alfredo has a PhD in Astrophysics and a Master's in Quantum Fields and Fundamental Forces from Imperial College London.

Space & Physics Editor

Alfredo has a PhD in Astrophysics and a Master's in Quantum Fields and Fundamental Forces from Imperial College London.View full profile

Alfredo has a PhD in Astrophysics and a Master's in Quantum Fields and Fundamental Forces from Imperial College London.

View full profile
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Valleys and lakes created by snowmelt have been discovered in Arabia Terra, photographed here in false color. NASA/JPL-Caltech/ASU


Today, Mars is a frigid red desert, but there was a time when the entire planet had an active water cycle. And according to new research, that period lasted longer than previously thought.

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A team of researchers led by Sharon Wilson, from the Smithsonian Institution and the University of Virginia, discovered that lakes and streams continued to flow on the Red Planet for over a billion years after a well-documented era of wet conditions. This finding could be crucial in our understanding of Mars and the potential for life there.

"We discovered valleys that carried water into lake basins," said Wilson in a statement. "Several lake basins filled and overflowed, indicating there was a considerable amount of water on the landscape during this time.”

The findings, reported in the Journal of Geophysical Research Planets, discuss stream-flows and associated lakes that could have been seasonal. They estimated the age of the region by looking at the number of craters and if the water features were there before or after the impacts.

The team estimated that these valleys and lakes were formed between 2 and 3 billion years ago, long after Mars is believed to have lost its atmosphere and become cold. Although the finding indicates flowing water, this is consistent with a frozen Mars.

"The rate at which water flowed through these valleys is consistent with runoff from melting snow," Wilson said. "These weren't rushing rivers. They have simple drainage patterns and did not form deep or complex systems like the ancient valley networks from early Mars."

These types of valleys appear in vast mid-latitude regions both north and south of the equator. These shallow valleys were part of a global cycle of water rather than a local system.

Our exploration of Mars requires understanding of the geological epochs of the Red Planet and how water shaped this now inhospitable environment. A lot of clues point to a water-rich world in the distant past, and perhaps it was like this long enough for some lifeforms to evolve.


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